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The National Deuteration Facility is providing deuterated cholesterol, an essential ingredient in lipid nanoparticles for the delivery of vaccines using mRNA, to academic and industry partners.

ANSTO’s user office in Melbourne offers access to the Australian Synchrotron, a world-class research facility with over 4,000 user visits per year. ANSTO seeks collaboration and partnerships with research organisations, scientific users and commercial users.

Scientists from the Walter and Eliza Hall Institute (WEHI) are using the unique immune system of the alpaca and techniques at the Australian Synchrotron as part of research using antibodies to disrupt COVID-19 viral entry into cells.

In early February, ANSTO was honoured to host the International Atomic Energy Agency (IAEA) National Liaison Officers Meeting and Sub Regional Approach to the Pacific Islands (SAPI) Programme, which focused on the development and delivery of the IAEA Technical Cooperation Programme in the Pacific.

Inspiring young women to be part of next generation of scientists.

In April 15, 1953, Australia entered the nuclear science arena, when the Atomic Energy Act came into effect. The Australian Atomic Energy Commission (AAEC) followed and in 1987 the AAEC evolved into the Australian Nuclear Science and Technology Organisation (ANSTO) as it’s known today.

Nuclear science is crucial to understanding our universe, our world and ourselves at the atomic level. If we can understand how atoms get together, interact, or can be best combined with other atoms, new, more efficient materials and drugs can be developed.

Pioneering work on materials for energy production, such as lithium ion batteries, has made ANSTO a centre of specialist capabilities and expertise.

More than 3,200 solar panels have been installed across the rooftops of the Australian Nuclear Science and Technology Organisation’s (ANSTO) Australian Synchrotron in Clayton, offsetting enough power to light up the whole MCG for more than five years.

Soft x-rays are generally understood to be x-rays in the energy range 100-3,000 eV. They have insufficient energy to penetrate the beryllium window of a hard x-ray beamline but have energies higher than that of extreme ultraviolet light.